Journal
GEOPHYSICAL RESEARCH LETTERS
Volume 27, Issue 2, Pages 157-160Publisher
AMER GEOPHYSICAL UNION
DOI: 10.1029/1999GL003632
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The 3D Plasma and Energetic Particle (3DP) instrument on the WIND spacecraft detected extremely cold solar wind electrons in the January 10-11, 1997 magnetic cloud, similar to 4 times lower temperature than any previously reported measurement. Detailed fits to the electron distributions show that the core electron temperature, T-ec, generally ranged from similar to 1 to 4.5 eV through the cloud, dropping to a low of similar to 0.7 eV in an unusually dense (n>similar to 150 cm(-3)) region in the trailing portion of the cloud. Due to the extremely low average electron temperature T-e and high density, the ions and electrons are collisionally coupled as confirmed by T-e=T-p, the first such observation in the solar wind. For most of the cloud the halo density is very low (n(eh)
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